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The Distance of the Gamma-ray Binary 1FGL J1018.6-5856

The recently discovered gamma-ray binary 1FGL J1018.6-5856 has a proposed optical/near-infrared (OIR) counterpart 2MASS 10185560-5856459. We present Stromgren photometry of this star to investigate its photometric variability and measure the reddening and distance to the system. We find that the gamma-ray binary has E(B-V) = 1.34 +/- 0.04 and d = 5.4^+4.6_-2.1 kpc. While E(B-V) is consistent with X-ray observations of the neutral hydrogen column density, the distance is somewhat closer than some previous authors have suggested.

preprint2011arXivOpen access
Vanessa J. NapoliM. Virginia McSwainAmber N. Marsh BoyerRachael M. Roettenbacher
astro-ph.HEastro-ph.SR
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Vanessa J. NapoliM. Virginia McSwainAmber N. Marsh BoyerRachael M. Roettenbacher

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